Fast spectral line calculations with the escape probability method and tests using synthetic observations of interstellar clouds

Open Access

Fig. 12

Estimated χ² for combined CS and C³⁴S observations of a BE sphere with M = 0.5 M_⊙ and T_kin = 10 K. The columns correspond to the assumed C³⁴S abundances (correct and with ±50% errors). The first row shows results for the J = 1 − 0 line, and each subsequent row adds one more rotational transition.

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